BEGIN:VCALENDAR VERSION:2.0 PRODID:-//CERN//INDICO//EN BEGIN:VEVENT SUMMARY:Modelling solar eruptive events from their onset to their propagat ion at 1 AU DTSTART;VALUE=DATE-TIME:20230510T101000Z DTEND;VALUE=DATE-TIME:20230510T102500Z DTSTAMP;VALUE=DATE-TIME:20240704T115654Z UID:indico-contribution-330@meetings.aip.de DESCRIPTION:Speakers: Antoine Strugarek ()\nIn the era of Solar Orbiter an d Parker Solar Probe\, we have now an unprecedented view on eruptive event s of the Sun\, from their onset to their propagation in the heliosphere. T hanks to the proximity of the probes to the Sun for at least part of their orbit\, we are currently acquiring more and more key data on the structur ing and the propagation of solar eruptive events\, as well as on the accel eration of particles at each stage of the eruption and propagation.\n\nI w ill report on an on-going modelling effort of solar eruptive events using the versatile PLUTO code within the STORMGENESIS project. I will present a full MHD effort to model idealised and realistic and eruptive active regi ons\, based on the initiation of the magnetic with both non-linear force-f ree and non force-free extrapolations. I will present very recent result o n the modelling of the eruption of active region #12241\, which is well re produced when using a non force-free initiation. Coupled to charged test-p articles under the gyrokinetic approximation\, and to the heating and cool ing associated with magnetic reconnection and radiative losses\, I will pr esent first results on the prediction for thermal and non-thermal emission from this active region. \n\nIn a second part\, I will show how the same simulation framework\, now using adaptive mesh refinement\, can be used to model the propagation of coronal mass ejections from their onset to their propagation up to 1 AU in a realistically structured solar wind. These re sults\, published recently in Regnault et al. (2023)\, allow to highlight the generic features of CMES and the simulation results compare very well with superposed-epochs analysis of hundreds of CMEs. In addition\, these s imulations point towards various rotation patterns of the CMEs that depend on their size and that happen during the initial stage of their propagati on within the Alfvén surface. These results warrant further analyses\, co upling the two set of simulations presented here to provide a complete pic ture of the energetics and of thermal and non-thermal emission of solar er uptive events.\n\nhttps://meetings.aip.de/event/24/contributions/330/ LOCATION:Haus H\, Telegrafenberg URL:https://meetings.aip.de/event/24/contributions/330/ END:VEVENT END:VCALENDAR